Dino Hunt

$4.00

by Jason Lie

Jurrasic park battles

In Jurassic Park Dinosaur Bat-tles, you take on the role of a government agent who has to rescue Harrison Manlyl's group of Junior Explorers from Isle Sorna (Site B) and stop the evil Ingen scientist Dr. Irene Corts from creating controllable dinosaurs with the experimental DinoVoc, using a DinoVoc stolen from

an abandoned lab that belonged to Corts.

The game features an isometric overworld and random RPG-style encounters. It is essentially the same as Jurassic Park Scan Com-mand, minus the need of the barcode scanner to progress. Since it is the same, both games will be mentioned here as the unused con-tent is essentially the same with a few exceptions. This map seems to either possibly be connected to the Cave in Area 3 where you rescue Kirby, or it's an early version of Area 3. Features a Dinosaur Nest interestingly. The dinosaur nest is actual-ly a separate graphic itself that appears on the map over the loca-tion, but this is where you would find it on the map.

Interestingly, the collision and tree maps are still in the game, so it may be possible to get the level up somehow. However, more re-search is needed. Anyway, here are the collision and tree maps. Among the related map objects for Area 4 is an unused image of a Camper similar to the one in Area 1. The reason why there's an an-imation is because map objects are invisible until you reach them, at which point they slowly fade into view. The Area 4 assets also contain a texture for the Camper's 3D model, but it's identical to the Camper's Area 1 texture. The Camper matches up perfectly in Area 4 to a spot usually occupied by not much other than trees CREDITS WWW.GOOGLE.COM/DINOSAUR BATTLES.

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steroids are minor planets, especially those of the inner Solar System. The larger ones have also been called planetoids. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disk of a planet and was not observed to have the characteristics of an active comet, but as minor planets in the outer Solar System were discovered, their volatile-based surfaces were found to resemble comets more closely and

so were often distinguished from traditional asteroids.[1][not in citation given] Thus the term as-teroid has come increasingly to refer specifically to the small bodies of the inner Solar System out to the orbit of Jupiter.[citation needed] They are grouped with the outer bodies—cen-taurs, Neptune trojans, and trans-Neptunian objects—as minor planets, which is the term preferred in astronomical circles.[2] In this article the term “asteroid” refers to the minor planets of the inner Solar System. There are millions of asteroids, many thought to be the shattered remnants of planetesimals, bodies within the young Sun’s solar nebula that never grew large enough to become planets.[3] The large majority of known asteroids orbit in the asteroid belt between the orbits of Mars and Jupiter, or are co-orbital with Jupiter (the Jupiter Trojans). However, oth-er orbital families exist with significant populations, including the near-Earth asteroids. Individual asteroids are classified by their characteristic spectra, with the majority falling into three main groups: C-type, S-type, and M-type. These were named after and are generally identified with carbon-rich, stony, and me-tallic compositions, respectively. Only one asteroid, 4 Vesta, which has a rela-tively reflective surface, is normally visible to the naked eye, and this only in very dark skies when it is favorably positioned. Rarely, small asteroids passing close to Earth may be visible to the naked eye for a short time.[4] As of September 2013, the Minor Planet Center had data on more than one million objects in the inner and outer Solar System, of which 625,000 had enough information to be given numbered designations.[5]

On 22 January 2014, ESA scientists reported the detection, for the first definitive time, of water vapor on Ceres, the largest object in the asteroid belt.[6] The detection was made by using the far-infrared abilities of the Herschel Space Observatory.[7] The finding is unexpected because comets, not asteroids, are typically con-sidered to “sprout jets and plumes”. According to one of the scientists, “The lines are becoming more and more blurred between comets and asteroids.”[A newly discovered asteroid is given a provisional designa-tion (such as 2002 AT4) consisting of the year of discovery and an alphanumeric code indicating the half-month of discovery and the sequence within that half-month. Once an asteroid’s orbit has been confirmed, it is given a number, and later may also be given a name (e.g. 433 Eros).

ASTROIDS

A

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The first asteroid to be discovered, Ceres, was found in 1801 by Giuseppe Piazzi, and was orig-inally considered to be a new planet.[note 1] This was followed by the discovery of other sim-ilar bodies, which, with the equipment of the time, appeared to be points of light, like stars, showing little or no planetary disc, though read-ily distinguishable from stars due to their appar-ent motions. This prompted the astronomer Sir William Herschel to propose the term “aster-

oid”,[15] coined in Greek as ἀστεροειδής asteroeidēs ‘star-like, star-shaped’,

from Ancient Greek ἀστήρ astēr ‘star, planet’. In the

early second half of the nineteenth centu-

ry, the terms “asteroid” and “planet” (not always qualified as “minor”) were still used interchangeably; for example, the Annual of Scientific Discovery for 1871,

page 316, reads “Professor J. Watson has been awarded by the Paris Academy of Sciences, the astronomical prize, Lalande foundation, for the discovery of eight new asteroids in one year. The planet Lydia (No. 110), discovered by M. Borelly at the Marseilles Observatory [...] M. Borelly had previously discovered two planets bearing the numbers 91 and 99 in the system of asteroids revolving between Mars and Jupiter Historical methods[edit]

Asteroid discovery methods have dramatically improved over the past two centuries.

In the last years of the 18th century, Baron Franz Xaver von Zach organized a group of 24 astronomers to search the sky for the missing planet predicted at

about 2.8 AU from the Sun by the Titius-Bode law, partly because of the discovery, by Sir William Herschel in 1781, of the planet Uranus at the distance predicted by the

law. This task required that hand-drawn sky charts be prepared for all stars in the zodia-cal band down to an agreed-upon limit of faintness. On subsequent nights, the sky would be

charted again and any moving object would, hopefully, be spotted. The expected motion of the missing planet was about 30 seconds of arc per hour, readily discerible. Manual methods of the 1900s

and modern reporting[edit]

Until 1998, asteroids were discovered by a four-step process. First, a region of the sky was photographed by a wide-field telescope, or astrograph. Pairs of photographs were taken, typically one hour apart. Multiple pairs could be taken over a series of days. Second, the two films or plates of the same region were viewed under a stereoscope. Any body in orbit around the Sun would move slightly between the pair of films. Under the stereo-scope, the image of the body would seem to float slightly above the background of stars. Third, once a moving body was identified, its location would be measured precisely using a digitizing microscope. The location would be measured relative to known star locationsThese first three steps do not constitute asteroid discovery: the observer has only found an appari-tion, which gets a provisional designation, made up of the year of discovery, a letter representing the half-month of discovery, and finally a letter and a number indicating the discovery’s sequential number. CREDITS WWW.WIKIPEDIA./ASTROIDS

SWIMING DINOSAURS

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ersons’ latest PhD research has produced some of the strongest evidence ever found that dinosaurs could paddle long dis-tances. Persons arrived at that conclusion after examining unusual claw marks on fossilized rocks found in China. Persons’

swimming-dinosaur study involved working with an inter-national team of researchers in China’s Szechuan Province. Persons determined that a series of claw marks found in now well-known dinosaur tracks were left by the tips of a two-legged dinosaur’s feet. “The dinosaur’s claw marks show it was swimming along in this river and just its tip-toes were touching bottom,” said Persons. The claw marks cover a distance of 15 metres, which the researchers say is

evidence of a dinosaur’s ability to swim with co-ordinated leg movements. Persons says the tracks were made by a carnivorous, two-legged dinosaur he estimates to have stood roughly one metre at the hip. The research was conducted with a team of paleontologists on the ground in China, but Persons says he and his fellow U of A dinosaur hunters don’t have to go far afield to make important discoveries—one of the reasons he decided to study at the university. “I don’t even have to leave the Edmonton city limits, and when I do, the fossil treasure trove in the Alberta badlands is less than a day’s leisurely drive away,” said Persons. Persons and his colleagues from the Szechuan Province fossil site will continue to analyze the dinosaurs’ swimming prowess with hopes that it will yield evidence related to today’s animals. In the meantime, Persons offers a few links paleontology has already established between life on Earth 65 million years ago and today. “Want to know why our pet dogs or livestock have limited colour vision? It’s because early mammals sacrificed cones for rods in their eyes so they could see better in the dark and better avoid dinosaurs. - See more at: http://uofa.ualberta.ca/news-and-events/newsarticles/2013/april/swimming-dino-saurs-help-researchers-track-evolution#st-hash.AiqlZ6q7.dpuf

“Want to understand the widespread success of modern flowering plants? Well, they evolved under the selective pressures of herbivorous dinosaurs. “Want to know where birds come from? Dinosaurs.” Per-sons was a co-author on the research, which was published April 8 in the journal Chinese Science Bulletin.

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CREDITS : http://uofa.ualberta.ca/

THIS IS A PICTURE OF A CARNATAURUS COME VISIT US